| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1781808 | Planetary and Space Science | 2011 | 5 Pages |
Abstract
The physics behind and the related conditions for these liquid waters to evolve and to exist, and possibly related consequences, are discussed. These calculations are mainly made in view of the possible presence of these sub-surface liquids in the upper surface of the present Mars.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
D. Möhlmann,